| Issue |
A&A
Volume 705, January 2026
|
|
|---|---|---|
| Article Number | A4 | |
| Number of page(s) | 11 | |
| Section | Astrophysical processes | |
| DOI | https://doi.org/10.1051/0004-6361/202556161 | |
| Published online | 19 December 2025 | |
Line-force-driven wind from a thin disk in a tidal disruption event
1
Shanghai Key Lab for Astrophysics, Shanghai Normal University, 100 Guilin Road, Shanghai 200234, China
2
Department of Physics and Chongqing Key Laboratory for Strongly Coupled Physics, Chongqing University, Chongqing 400044, PR China
3
Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China
4
Polar Research Institute of China, 451, Jinqiao Road, Pudong, Shanghai 200136, China
5
Department of Physics, Nanjing Normal University, Nanjing 210023, China
★ Corresponding authors: This email address is being protected from spambots. You need JavaScript enabled to view it.
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Received:
29
June
2025
Accepted:
19
October
2025
Context. Winds from the accretion disk in tidal disruption events (TDEs) play a key role in determining their observed emission. While winds from the super-Eddington accretion phase in TDEs have recently been studied, the properties of winds from the sub-Eddington accretion disk remain unclear.
Aims. We aimed to investigate the properties of winds from the circularized sub-Eddington accretion disk in TDEs and study the line-force-driven accretion disk wind.
Methods. We performed two-dimensional hydrodynamic simulations using the PLUTO code to study the line-force-driven wind from the circularized accretion disk around a 106 solar mass black hole in TDEs.
Results. We find that although the disk is very small in TDEs, a strong wind can be driven by line force when the disk has a luminosity greater than 20% of the Eddington luminosity. The maximum velocity of the wind can reach up to 0.3 times the speed of light. The kinematic power of wind ranges from 1 − 6% of the Eddington luminosity.
Conclusions. Strong winds can be driven by line force from the thin disk around a 106 solar mass black hole in TDEs. We briefly discuss the possible radio emission from the shock when the wind collides with the surrounding medium.
Key words: accretion, accretion disks / black hole physics
© The Authors 2025
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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